We measure the clustering of DES year 1 galaxies that are intended to be combined with
weak lensing samples in order to produce precise cosmological constraints from the joint …

In this work, we present the galaxy clustering measurements of the two DES lens galaxy
samples: a magnitude-limited sample optimized for the measurement of cosmological …

We present cosmological constraints from the Dark Energy Survey (DES) using a combined
analysis of angular clustering of red galaxies and their cross-correlation with weak …

We present the calibration of the Dark Energy Survey Year 3 (DES Y3) weak lensing (WL)
source galaxy redshift distributions n (z) from clustering measurements. In particular, we …

We present galaxy-galaxy lensing measurements from 1321 sq. deg. of the Dark Energy
Survey (DES) Year 1 (Y1) data. The lens sample consists of a selection of 660,000 red …

We study the effect of magnification in the Dark Energy Survey Year 3 analysis of galaxy
clustering and galaxy–galaxy lensing, using two different lens samples: a sample of …

We present the first cosmology results from large-scale structure using the full 5000 deg 2 of
imaging data from the Dark Energy Survey (DES) Data Release 1. We perform an analysis …

We constrain cosmological parameters and galaxy-bias parameters using the combination
of galaxy clustering and galaxy-galaxy lensing measurements from the Dark Energy Survey …

Several dark energy experiments are available from a single large-area imaging survey and
may be combined to improve cosmological parameter constraints and/or test inherent …

We present cosmological results from a combined analysis of galaxy clustering and weak
gravitational lensing, using 1321 deg 2 of griz imaging data from the first year of the Dark …